松辽盆地南部岩石圈地幔变形特征及各向异性分析——来自橄榄岩包体的约束

SKS测量结果显示松辽盆地快波方向分布较为复杂, 由于缺乏深部岩石变形资料约束, 制约了地震波各向异性成因解释。本文通过对松辽盆地南部双辽地区橄榄岩包体进行详细的岩石学、地球化学、显微结构、各向异性研究, 结果显示双辽地区橄榄岩包体的平衡温度为893~1152℃, 来源于岩石圈地幔。橄榄岩中橄榄石的晶格优选方位(CPO)类型主要为A型、D型和AG型, 其中, AG型和D型CPO可能形成于西太平洋板块向欧亚大陆俯冲回撤导致的岩石圈变形, AG型橄榄石CPO也可能形成于熔体存在下的橄榄石变形。基于CPO计算获得的橄榄岩包体全岩V_P各向异性(AV_P)为4.79%~11.80%, 最大剪切波各向异性(AV_Smax)为3.13%~7.93%。结合地球物理测量结果, 推断松辽盆地南部复杂的SKS各向异性的主要贡献可能来源于面理陡倾或直立的岩石圈地幔。

     

松辽盆地中央坳陷区中—新生代岩石圈厚度演化

岩石圈厚度演化为揭示深部动力学过程提供依据和重要信息。本文通过恢复松辽盆地中央凹陷区典型单井的热历史,利用实测的热物性参数和前人所确定的地壳分层结构,基于地热学相关理论计算了松辽盆地中—新生代主要地质时期的“热”岩石圈厚度。研究表明,松辽盆地中央凹陷区热流演化有两个阶段：1）晚白垩世逐渐升温阶段,此期间热流逐渐增加,最终在白垩纪末期达到最大热流值;2）新生代以来的热流衰退阶段,此阶段构造活动相对稳定,大地热流在此期间逐渐减少,现今热流平均为78.2 mW/m²。松辽盆地岩石圈厚度在早白垩世为42 km左右,白垩世末期降低至36 km左右,现今岩石圈厚度增加至55 km。这主要是由于在侏罗纪—白垩纪时期,中国东部大陆岩石圈整体处于东西拉张的环境中,地壳和岩石圈伸展减薄,导致白垩纪末期岩石圈减薄,此后盆地整体处于拗陷构造发育期,岩石圈再次增厚至现今的55 km。本文的研究成果初步揭示了松辽盆地中—新生代岩石圈演化的过程,为松辽盆地深部动力学过程提供依据,并具有重要的科学意义。

     

The evolution of lithospheric mantle beneath the Kalahari Craton and its margins

The compositional structure and thermal state of the subcontinental lithospheric mantle (SCLM) beneath the Kalahari Craton and the surrounding mobile belts have been mapped in space and time using >3400 garnet xenocrysts from >50 kimberlites intruded over the period 520–80 Ma. The trace-element patterns of many garnets reflect the metasomatic refertilisation of originally highly depleted harzburgites and lherzolites, and much of the lateral and vertical heterogeneity observed in the SCLM within the craton is the product of such metasomatism. The most depleted, and possibly least modified, SCLM was sampled beneath the Limpopo Belt by early Paleozoic kimberlites; the SCLM beneath other parts of the craton may represent similar material modified by metasomatism during Phanerozoic time. In the SW part of the craton, the SCLM sampled by “Group 2” kimberlites (>110 Ma) is thicker, cooler and less metasomatised than that sampled by “Group 1” kimberlites (mostly ≤95 Ma) in the same area. Therefore, the extensively studied xenolith suite from the Group 1 kimberlites probably is not representative of primary Archean SCLM compositions. The relatively fertile SCLM beneath the mobile belts surrounding the craton is interpreted as largely Archean SCLM, metasomatised and mixed with younger material during Paleoproterozoic to Mesoproterozoic rifting and compression. This implies that at least some of the observed secular evolution in SCLM composition worldwide may reflect the reworking of Archean SCLM. There are strong correlations between mantle composition and the lateral variations in seismic velocity shown by detailed tomographic studies. Areas of relatively low Vp within the craton largely reflect the progressive refertilisation of the Archean root during episodes of intraplate magmatism, including the Bushveld (2 Ga) and Karroo (ca. 180 Ma) events; areas of high Vp map out the distribution of relatively less metasomatised Archean SCLM. The relatively low Vp of the SCLM beneath the mobile belts around the craton is consistent with its fertile composition. The seismic data may be used to map the lateral extent of different types of SCLM, taking into account the small lateral variations in the geotherm identified using the techniques described here.     

Late Pleistocene crustal uplift and gravity anomaly in the eastern part of Kyushu, Japan, and its geophysical implications

The Miyazaki Plain, eastern part of Kyushu, Japan, is characterized by both significant negative gravity anomalies and aseismic crustal uplifting (1 mm/year) in the Late Pleistocene and Holocene. We examine the relationship between these two phenomena, which may provide important constraints on the interaction between the collision and/or subduction of the Kyushu-Palau Ridge and the forearc. We estimate the mass deficiency below 11-km depth by using the gravity anomalies and P-wave velocity structure of the upper crust. The onset of the load accumulation, 0.5–0.4 Ma, is inferred from the movement of the fluvial terraces considering the tephrochronology. The loading history is assumed to be a linear function of time. We evaluate the crustal rebound by assuming a viscoelastic plate deformation with an underplating load existing at 20- or 30-km depth. The predicted crustal movement for models with a lithospheric (crustal) viscosity of 10²³–10²⁴ Pa s can explain the observed altitudes of the shoreline of the marine terraces formed at the Last Interglacial of about 125 kyr BP and the middle Holocene of 5–6 kyr BP. Although we cannot restrict the origin of the buoyant body, the subduction of the Kyushu-Palau Ridge, remnant arc associated with back-arc opening of the Shikoku Basin, may be related to the buoyancy for the uplifting region examined here. On the other hand, the buoyant body off the Miyazaki Plain probably plays an important role in the interaction between the subducting oceanic slab and the overriding forearc crust. Thus, the observed lateral variation of the interplate coupling on the convergent boundary along the Nankai Trough may be attributed to the existence of the buoyant body.     

Seismic crustal structure between the Transylvanian Basin and the Black Sea, Romania

In order to study the lithospheric structure in Romania a 450 km long WNW–ESE trending seismic refraction project was carried out in August/September 2001. It runs from the Transylvanian Basin across the East Carpathian Orogen and the Vrancea seismic region to the foreland areas with the very deep Neogene Focsani Basin and the North Dobrogea Orogen on the Black Sea. A total of ten shots with charge sizes 300–1500 kg were recorded by over 700 geophones. The data quality of the experiment was variable, depending primarily on charge size but also on local geological conditions. The data interpretation indicates a multi-layered structure with variable thicknesses and velocities. The sedimentary stack comprises up to 7 layers with seismic velocities of 2.0–5.9 km/s. It reaches a maximum thickness of about 22 km within the Focsani Basin area. The sedimentary succession is composed of (1) the Carpathian nappe pile, (2) the post-collisional Neogene Transylvanian Basin, which covers the local Late Cretaceous to Paleogene Tarnava Basin, (3) the Neogene Focsani Basin in the foredeep area, which covers autochthonous Mesozoic and Palaeozoic sedimentary rocks as well as a probably Permo-Triassic graben structure of the Moesian Platform, and (4) the Palaeozoic and Mesozoic rocks of the North Dobrogea Orogen. The underlying crystalline crust shows considerable thickness variations in total as well as in its individual subdivisions, which correlate well with the Tisza-Dacia, Moesian and North Dobrogea crustal blocks. The lateral velocity structure of these blocks along the seismic line remains constant with about 6.0 km/s along the basement top and 7.0 km/s above the Moho. The Tisza-Dacia block is about 33 to 37 km thick and shows low velocity zones in its uppermost 15 km, which are presumably due to basement thrusts imbricated with sedimentary successions related to the Carpathian Orogen. The crystalline crust of Moesia does not exceed 25 km and is covered by up to 22 km of sedimentary rocks. The North Dobrogea crust reaches a thickness of about 44 km and is probably composed of thick Eastern European crust overthrusted by a thin 1–2 km thick wedge of the North Dobrogea Orogen.     

Constraints from Moho geometry and crustal thickness on the geodynamic origin of the Vrancea Seismogenic Zone (Romania)

Reprocessing of industry deep seismic reflection data (Ramnicu Sarat and Braila profiles) from the SE Carpathian foreland of Romania provides important new constraints on geodynamic models for the origin of the intermediate depth Vrancea Seismogenic Zone (VSZ). Mantle (70–200 km) earthquakes of the VSZ are characterized by high magnitudes (greater than 6.5), frequent occurrence rates (approximately 25 years), and confinement in a very narrow (30 × 70 × 200 km³) near vertical zone atypical for a Wadati–Benioff plane, located in front of the orogen. These two deep (20 s) seismic reflection profiles (70 km length across the foreland) reveal (1) a high-amplitude, gently east-dipping reflection across most of the section from what we interpret to be the Moho at  15 s (40–42 km) on the Ramnicu Sarat line to  16 s (47–48 km) on the Braila line, (2) a thick sedimentary cover increasing in thickness from east (1 s;  800 m) to west (7.5 s; 14 km), (3) an eastward increase in crustal thickness from 38 km (near VSZ) to  45 km, (4) seismic and topographic evidence for a newly imaged, possibly seismically active basement fault with a surface offset of 30 m observed on the Ramnicu Sarat line, (5) a lack of notable west-dipping structures in the crust and across the Moho, and (6) variable displacements on Peceneaga–Camena Fault of  5 km at Moho and  200 m at the basement–sedimentary cover contact.These observations appear to argue against recent models for west-dipping subduction of oceanic lithosphere at or in the vicinity of the Vrancea Seismogenic Zone given the lack of west-dipping fabrics in the lower crust and across the crust–mantle boundary. Consequently, one possible explanation for the geodynamic origin of VSZ could be partial delamination of the continental lithosphere in an intra-plate setting along a sub-horizontal lithospheric interface in the Carpathian hinterland that likely involves remnant lithospheric coupling between the crust and uppermost mantle in the foreland.     

The crustal structure of the Guayana Shield, Venezuela, from seismic refraction and gravity data

We present results from a seismic refraction experiment on the northern margin of the Guayana Shield performed during June 1998, along nine profiles of up to 320 km length, using the daily blasts of the Cerro Bolívar mines as energy source, as well as from gravimetric measurements. Clear Moho arrivals can be observed on the main E–W profile on the shield, whereas the profiles entering the Oriental Basin to the north are more noisy. The crustal thickness of the shield is unusually high with up to 46 km on the Archean segment in the west and 43 km on the Proterozoic segment in the east. A 20 km thick upper crust with P-wave velocities between 6.0 and 6.3 km/s can be separated from a lower crust with velocities ranging from 6.5 to 7.2 km/s. A lower crustal low velocity zone with a velocity reduction to 6.3 km/s is observed between 25 and 25 km depth. The average crustal velocity is 6.5 km/s. The changes in the Bouguer Anomaly, positive (30 mGal) in the west and negative (−20 mGal) in the east, cannot be explained by the observed seismic crustal features alone. Lateral variations in the crust or in the upper mantle must be responsible for these observations.     

3-D crustal structure of the extensional Granada Basin in the convergent boundary between the Eurasian and African plates

Three-dimensional P and S wave velocity models of the crust under the Granada Basin in Southern Spain are obtained with a spatial resolution of 5 km in the horizontal direction and 2 to 4 km in depth. We used a total of 15407 P and 13704 S wave high-quality arrival times from 2889 local earthquakes recorded by both permanent seismic networks and portable stations deployed in the area. The computed P and S wave velocities were used to obtain three-dimensional distributions of Poisson's ratio (σ) and the porosity parameter (V_p×V_s). The 3-D velocity images show strong lateral heterogeneities in the region. Significant velocity variations up to ±7% in P and S velocities are revealed in the crust below the Granada Basin. At shallow depth, high-velocity anomalies are generally associated with Mesozoic basement, while the low-velocity anomalies are related to the neogene sedimentary rocks. The south–southeastern part of the Granada Basin exhibits high σ values in the shallowest layers, which may be associated with saturated and unconsolidated sediments. In the same area, V_p×V_s is high outside the basin, indicating low porosity of the mesozoic basement. A low-velocity zone at 18-km depth is found and interpreted as a weak–ductile crust transition that is related to the cut-off depth of the seismic activity. In the lower crust, at 34-km depth, a clear slow V_p and V_s anomalous zone may indicate variations in lithology and/or with the rigidity of the lower crust rocks.     

Three-dimensional earthquake locations and upper crustal structure of the Sannio-Matese region (southern Italy)

The Sannio-Matese region is one of the most seismically active regions of Italy and has been struck by large historical earthquakes. At present, the area is characterized by low magnitude background seismicity and small seismic sequences following M4 main events. In this paper, we show Vp and Vp/Vs models and 3D locations for a complete set of earthquakes occurring in the period 1991–2001. We observe a significant crustal heterogeneity, with large scale east-verging high Vp fault-related-folds, stacked by the Pliocene compression. The relocated earthquakes cluster along a 70° east-dipping, NW-striking plane located at the border of the high Vp thrust units. Normal fault earthquakes related to the young and active extension occur within these high Vp zones, interpreted as high strength material. We expect large future earthquakes to occur within these high Vp zones actually characterized by low magnitude seismicity at their borders.     

宽角反射、折射地震数据与重力数据综合解释龙门山及邻近地区地壳结构

青藏高原东部的隆升机制一直都是地学界的研究热点,研究学者们提出和发展了多种岩石圈变形模型,而存在多种模型的主要原因之一是对青藏高原东部地壳及岩石圈结构认识不足。本文主要针对SinoProbe-02项目横跨龙门山断裂带、全长400多公里的宽角、折射地震数据及重力数据进行联合反演和综合解释。研究结果表明,龙门山及邻近地区地壳结构可明确划分为上地壳、中地壳和下地壳。上地壳上层为沉积层,龙门山断裂带以西大部分区域被三叠纪复理岩覆盖,而在龙日坝断裂与岷江断裂之间出现了密度为2.7g/cm³的高速异常体;向东靠近龙门山地区,沉积层厚度逐渐减薄。中地壳速度变化不均一,而且变形强烈;若尔盖盆地和龙门山断裂带下方出现明显低速带;中地壳在龙门山西侧厚度加厚,在岷江断裂下方和四川盆地靠近龙门山断裂带地区附近厚度达到最大。莫霍面整体深度从东往西增厚,最厚可达56 km。本次研究得到的地壳结构和密度分布分析结果表明现有的地壳厚度和物质组成不足以支撑龙门山及邻近地区目前所达到的隆升高度,因此四川盆地刚性基底西缘因挤压作用产生的弯曲应力也是该地区抬升的重要条件之一。     

The major features of the crustal structure in north-eastern Venezuela from deep wide-angle seismic observations and gravity modelling

Venezuela is located on the plate boundary zone between the South American continent and the Caribbean plate. A relative movement of 2 cm/year is accommodated by a system of strike–slip faults running from the Andes to the Gulf of Paria. The Interior Range, a moderate-height mountain range, separates the Oriental Basin from the Caribbean. To the south, predominantly Precambrian rocks are outcropping in the Guayana Shield south of the Orinoco River. Results of deep wide-angle seismic measurements for the region were obtained during field campaigns in 1998 (ECOGUAY) for the Guayana Shield and in 2001 (ECCO) for the Oriental Basin. The total crustal thickness decreases from 45 km beneath the Guayana Shield, to 39 km at the Orinoco River, and 36 km close to El Tigre, in the center of the Oriental Basin. The average crustal velocity decreases in the same sense from 6.5 to 5.95 km/s. Detailed information was obtained on the velocity distribution within the Oriental Basin. Velocities are as low as 2.2 km/s for the uppermost 2 km, 4.5 km/s down to 4 km in depth, and a maximum depth of 13 km was derived for material with seismic velocities up to 5.9 km/s, interpreted as the base of the sedimentary basin. A gravimetric model confirms the structures derived from the seismic data. Discrete increases in sedimentary thickness along the basin may be associated to extension processes during the passive margin phase in the Cretaceous, or during earlier extension phases.     

Asymmetry in oceanic crustal structure of the South China Sea basin and its implications on mantle geodynamics

ABSTRACT

We investigated the oceanic crustal structure and lithospheric dynamics of the South China Sea (SCS) basin through a comprehensive analysis of residual gravity anomaly and bathymetry combined with seismic constraints and interpretation from geodynamic modelling. We first calculated the residual mantle Bouguer anomaly (RMBA) of the oceanic crustal regions of the SCS by removing from free-air gravity anomaly the predicted gravitational attractions of water-sediment, sediment-crust, and crust-mantle interfaces, as well as the effects of lithospheric plate cooling, using the latest crustal age constraints including IODP Expedition 349 and recent deep-tow magnetic surveys. We then calculated models of the gravity-derived crustal thickness and calibrated them using the available seismic refraction profiles of the SCS. The gravity-derived crustal thickness models correlate positively with seismically determined crustal thickness values. Our analysis revealed that the isochron-averaged RMBA are consistently more negative over the northern flank of the SCS basin than the southern conjugate for magnetic anomaly chrons C8n (~25.18 Ma) to C5Dn (~17.38 Ma), implying warmer mantle and/or thicker crust over much of the northern flank. Computational geodynamic modelling yielded the following interpretations: (1) Models of asymmetric and variable spreading rates based on the relatively high-resolution deep-tow magnetic analysis would predict alternating thicker and thinner crust at the northern flank than the southern conjugate, which is inconsistent with the observed systematically thicker crust on the northern flank. (2) Models of episodic southward ridge jumps could reproduce the observed N-S asymmetry, but only for crustal age of 23.6–20 Ma. (3) Southward migration of the SCS ridge axis would predict slightly thinner crust at the northern flank, which is inconsistent with the observations. (4) Models of higher mantle temperatures of up to 25–50°C or >2% less depleted mantle sources on the northern flank could produce large enough anomalies to explain the observed N-S asymmetries.     

青藏高原东缘地壳上地幔结构及其动力学意义

本文综述了我们在青藏高原东缘实施的垂直切过龙门山断裂带宽频带地震探测的研究成果,揭示了研究区复杂的地壳上地幔结构,结果表明松潘-甘孜地块与四川盆地西缘莫霍面深度为58 km与40 km±,在龙门山断裂带下方存在约15 km的莫霍面错断; 松潘-甘孜与龙门山断裂带域地壳纵横波速度比Vp/Vs比值远大于173,预示着粘性下地壳流或基性/超基性物质的存在。探讨了研究区强烈的盆山之间以及深部不同层圈之间的相互作用,推断四川盆地对青藏高原东缘软流圈驱动的物质东向逃逸阻挡作用可能深达整个上地幔。     

南海张裂过程及其对晚中生代以来东南亚构造的启示——IODP建议书735-Full介绍

南海的形成揭示了大陆边缘张裂和盆地形成的复杂模式,尽管已经进行了广泛研究,但是关于基底岩石和深海盆沉积层的精确年代数据还很缺乏,这使得对南海张裂年代的估计存在很大的误差,对张裂机制和历史的各种假设没有得到验证.同时只有对南海的张裂过程有了精确地分析与刻画,才能更好地理解西太平洋边缘海盆地的形成以及它们在印支块体受印度-欧亚板块碰撞而向东南挤出、青藏高原隆升中可能起到的作用.2009年正式提交的国际综合大洋钻探计划(IODP)建议书735-Full建议在南海深海盆内的4个站位上实施钻探.这4个站位分布在南海盆地4个不同的次级构造单元上(南海东北部、西北次海盆、东部次海盆和西南次海盆),这样的站位设计会确保完成本建议书的整体研究目标,即揭示南海的张裂历史和它对晚中生代以来东南亚构造的启示.位于南海盆地最东北部的站位有助于确定该区域地壳的属性和验证古南海是否存在,位于西北次海盆的站住可能会提供南海的最早张裂年代,另外2个分别位于东部次海盆和西南次海盆的站位将重点确定2个次海盆的绝对年龄、基底矿物成分与磁化率以及2个次海盆的相对张裂次序.这些站位的水深大约在2 910～4 400 m,钻探深度预计到海底以下大约700～2 200 m,总的钻透深度为5 959 m,其中5 359 m穿透沉积层,另外600 m或400 m钻入基底.所有这些站位的位置是由已有的地球物理观测数据所确定,目前计划收集更多的地质与地球物理数据以满足IODP对井位调查数据的要求.     

郯庐断裂带张八岭隆起南段晚中生代侵入岩地球化学及其对岩石圈减薄的指示

本文报道了郯庐断裂带张八岭隆起南段晚中生代侵入岩的主量元素、微量元素及Sr-Nd-Pb同位素特征。研究区侵入岩为一套铝和硅均过饱和的、准铝质向过铝质过渡的岩浆岩,具有富碱、富钾的特征,可根据侵位时间和地球化学特征将张八岭隆起南段侵入岩划分为四类:早期、中早期、中晚期和晚期。早期和中早期侵入岩富集大离子亲石元素(LILE)和轻稀土元素(LREE),相对亏损重稀土元素(HREE),为一套埃达克质的钙碱性二长花岗岩,分别具有正Eu异常和无Eu异常;中晚期和晚期侵入岩富集LILE,亏损Ba、Sr,具有负的Eu异常,是一套碱性A型花岗岩。中晚期和晚期侵入岩与早期和中早期侵入岩相比,具有更低的CaO、MgO、Fe₂O^T₃、Al₂O₃、REE含量、(La/Yb)_N值和更高的Eu负异常和SiO₂含量。Sr-Nd-Pb同位素特征显示,张八岭隆起南段侵入岩岩浆主要来源于华北克拉通下地壳。早期岩浆包含少量的富集地幔端元,而晚期岩浆则为更浅的地壳源区。先期的埃达克质岩代表了该处岩石圈伸展活动的开始阶段,而后期的A型花岗岩则代表了岩石圈强烈伸展的时间。研究表明,岩浆侵位过程中没有经历明显的中、上地壳混染,岩浆源区经历了不同程度的部分熔融,并经历了分离结晶作用。随岩浆侵位时间的变化,岩浆源区的残留相明显不同,由早到晚从石榴子石到斜长石再向角闪石过渡,且岩浆源区逐渐变浅。岩浆演化规律暗示岩浆活动的深部动力学过程为:华北克拉通岩石圈底部的逐渐减薄造成了软流圈顶面抬升,导致岩石圈内热流升高,化学作用逐渐加强,从而出现了不同深度的下地壳源区部分熔融。与远离断裂带的克拉通内部相比,郯庐断裂带具有更强烈的岩石圈伸展程度、侵入岩具有更浅的岩浆源区、岩浆源区具有更强烈的演化程度和更高程度的部分熔融。一系列的证据进一步均证明郯庐断裂带是岩石圈减薄中的强减薄带。     

北萨哈林盆地的热演化特征与影响因素

北萨哈林盆地作为俄罗斯远东地区最大的含油气盆地,其热流分布和演化过程对油气勘探有重要意义。本文通过单井和区域热流分析,恢复了北萨哈林盆地和鄂霍茨克海域各时期热流值的分布范围;对沉积盆地热演化各期次进行数值模拟,改进了简单沉降模型,使其适用于弧后拉分盆地;利用EASY%Ro 方法对热演化过程进行恢复,并与理论计算的热流值进行对比分析。研究表明,北萨哈林盆地各时期热流分布极为不均,热演化可以分成两个阶段：1） 古近纪,盆地内陆和海域具有各自的热流中心,其热演化过程相对独立;2） 晚渐新世后,盆地受弧后拉张和断裂剪切的共同作用,热流范围发生改变,构造拼合带成为新的热流中心。本文认为岩浆活动强弱和沉降速率差异是造成该现象的内因和外因。     

Deep structure of the northeastern Japan arc and its implications for crustal deformation and shallow seismic activity

Seismic tomography studies in the northeastern Japan arc have revealed the existence of an inclined sheet-like seismic low-velocity and high-attenuation zone in the mantle wedge at depths shallower than about 150 km. This sheet-like low-velocity, high-attenuation zone is oriented sub-parallel to the subducted slab, and is considered to correspond to the upwelling flow portion of the subduction-induced convection. The low-velocity, high-attenuation zone reaches the Moho immediately beneath the volcanic front (or the Ou Backbone Range) running through the middle of the arc nearly parallel to the trench axis, which suggests that the volcanic front is formed by this hot upwelling flow. Aqueous fluids supplied by the subducted slab are probably transported upward through this upwelling flow to reach shallow levels beneath the Backbone Range where they are expelled from solidified magma and migrate further upward. The existence of aqueous fluids may weaken the surrounding crustal rocks, resulting in local contractive deformation and uplift along the Backbone Range under the compressional stress field of the volcanic arc. A strain-rate distribution map generated from GPS data reveals a notable concentration of east–west contraction along the Backbone Range, consistent with this interpretation. Shallow inland earthquakes are also concentrated in the upper crust of this locally large contraction deformation zone. Based on these observations, a simple model is proposed to explain the deformation pattern of the crust and the characteristic shallow seismic activity beneath the northeastern Japan arc.     

准噶尔盆地南缘晚古生代双峰式火山岩成因机制及其地球动力学背景

准噶尔盆地南缘晚古生代双峰式火山岩组合以玄武岩和英安斑岩的伴生出现为特征。锆石LA-ICP-MS U-Pb定年结果显示,英安斑岩和玄武岩的结晶年龄分别为298±2 Ma和297~304 Ma。在地球化学组成上,英安斑岩样品富SiO_2、Al_2O_3和Na_2O,相对于原始地幔富集Th和LREE,明显亏损Nb、Ta和Ti等高场强元素;而玄武岩样品相对于原始地幔明显富集Th、LREE、Zr和Hf等,明显亏损Nb、Ta和Ti。全岩Sr-Nd同位素研究结果显示,英安斑岩样品(~(87)Sr/~(86)Sr)t值为0.705,εNd(t)值分布在+6.5~+11之间,而玄武岩样品的(~(87)Sr/~(86)Sr)t值为0.704,εNd(t)值分布在+7.5~+8.4之间。这些特征指示玄武岩和英安斑岩应分别起源于相对亏损的地幔源区和新生地壳组分的部分熔融。综合野外地质、岩石学、地球化学和同位素地质学等多方面的资料,可以确定准南地区玄武岩和英安斑岩并非同源岩浆作用的产物。其中,玄武岩应起源于亏损地幔的部分熔融,并且岩浆在上升侵位过程中经历了一定程度的陆壳混染。英安斑岩的形成与玄武质岩浆的底侵导致新生地壳组分的部分熔融有关。结合区域上已有的研究成果,认为至少从早二叠世(~298 Ma)开始,天山地区已经进入后碰撞阶段,区域构造体制开始由挤压转向伸展。     

复杂储层识别的地震反演方法及其在塔木察格盆地的应用

随着油气藏勘探开发程度的加深,准确识别复杂储层变得愈发重要,地震反演已成为储层预测的核心技术.本文对蒙占国塔木察格盆地南部凹陷1 800 km2地震资料进行波阻抗反演研究,研究工作包括测井曲线的标准化校正、地质框架模型的准确建立及其它反演参数的正确选取.波阻抗反演结果为研究沉积相划分、砂体空问展布的认识提供了可靠依据,在一定程度上解决了该区主要日的层南屯组沉积物源多、相变快和在地震剖面上无法追踪的问题.     

鄂尔多斯盆地早白垩世构造热事件形成动力学背景及其对油气等多种矿产成藏（矿）期的控制作用

华北克拉通中西部中生代晚期早白垩世是否存在岩石圈减薄是地学界普遍关注的重大地质问题。本文在作者多年来对鄂尔多斯盆地构造热演化史研究的基础上,充分收集了近年来前人研究的成果及进展,对鄂尔多斯盆地现今地温场、地壳结构、构造热事件、深部热岩石圈厚度、早白垩世火成岩活动期次、构造热事件形成机理及构造热事件与多种矿产成藏成矿关系方面进行探讨。鄂尔多斯盆地现今地温梯度及大地热流中等,属中温型盆地,现今地温场受现今地壳、岩石圈厚度较厚控制。通过对构造背景、古地温恢复、火成岩活动及热岩石圈厚度恢复等资料分析发现早白垩世太行山以西的山西地块及鄂尔多斯盆地处于拉张背景,早白垩世地温梯度高,存在古地温异常及热事件。早白垩世鄂尔多斯盆地热岩石圈厚度明显较现今岩石圈厚度薄,表明华北克拉通中生代晚期以来岩石圈减薄的西界可推到鄂尔多斯盆地。华北克拉通中西部鄂尔多斯盆地周缘、华北克拉通中部山西地块、华北克拉通中西部南缘早白垩世火成岩形成时间相同,岩浆侵入和喷出的时代主要集中在138～108Ma,反映在燕山晚期早白垩世华北克拉通中西部存在一期较为强烈的热事件。火成岩地球化学分析表明火成岩来源为地幔,反映岩石圈处于拉张背景。早白垩世热事件发生的时间与华北克拉通岩石圈减薄的峰期年龄相一致,表明华北克拉通岩石圈减薄作用在华北克拉通中西部广泛存在。早白垩世构造热事件发生的根本原因在于鄂尔多斯盆地岩石圈深部热活动增强,深部软流圈物质上涌,岩石圈厚度减薄。通过对油气、煤、铀等金属矿产成矿(藏)时代与热事件的对应关系分析发现鄂尔多斯盆地油气、煤、铀矿产及华北克拉通中西部金属矿产的形成受控于早白垩世构造热事件及岩石圈拉张减薄的深部热背景,主要成藏(矿)期均为早白垩世,成藏、成矿具有爆发式及同时性特点。